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Yes, the equation p2 = a3, where p is a planet's orbital period in years and a is the planet's average distance from the Sun in AU. This equation allows us to calculate the mass of a distance object if we can observe another object orbiting it and measure the orbiting object's orbital period and distance.

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Q: I used Newton's version of Kepler's third law to calculate Saturn's mass from orbital characteristics of its moon Titan?
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